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MER2 Pancam Calibrated Data Collection
This collection contains derived IOF images from the Panoramic Cameras (Pancam) on the Mars Exploration Rover 2 (Spirit). These products were produced by the Pancam Science Team. -
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MER1 Pancam Calibrated Data Collection
This collection contains calibrated images from the Panoramic Cameras (Pancam) on the Mars Exploration Rover 1 (Opportunity). These products were produced by the Pancam Science Team. -
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Roberts Eros Ponds Catalog V1.1
This data set contains two tables describing the size and location of ponded deposits on asteroid 433 Eros. Both tables contain the same pond information, but one is presented in the format required for ingestion by a publicly available 3D visualization application, the Small Body Mapping Tool (Ernst et al., 2018; http://sbmt.jhuapl.edu). -
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Mars Target Encyclopedia MER-2 Collection
MER-2 collection for the Mars Target Encyclopedia bundle -
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Arizona State University Ronald Greeley Center for Planetary Studies - The Ronald Greeley 35mm Slide Collection, The Jovian System, The Jovian System Bodies and Miscellaneous Objects
This collection, included in document_jovian_system_and_misc, consists of 245 digitized 35mm slides of Jovian System bodies and miscellaneous objects. Slides are divided into two databases, diagrams and photos, but are inventoried as a single collection. Information about each photograph, including location, description, and mission, are in the document_database in jovian_system_and_misc_diagram_database.pdf and jovian_system_and_misc_photo_database.pdf. The photographs and documentation are from the Dr. Ronald Greeley archive at the Arizona State University Ronald Greeley Center for Planetary Studies, Tempe, Arizona. -
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Cassini ISS Global Maps of Jupiter and Saturn Derived XML Schema Collection
Cassini ISS Global Maps of Jupiter and Saturn -
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data collection for the "GASKELL DIONE SHAPE MODEL" bundle
This is the data collection for the gaskell.dione.shape-model bundle. The shape model of Dione derived by Robert Gaskell from Cassini images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on July 23, 2012. Vertex-facet versions of the models are also provided. -
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Document collection for Arizona State University Ronald Greeley Center for Planetary Studies - The Ronald Greeley 35mm Slide Collection, The Jovian System, Ganymede
This collection, included in document_ganymede, consists of 108 digitized 35mm slides primarily of Ganymede, Galilean Satellite of Jupiter, and other related bodies. Slides are divided into two databases, diagrams and photos, but are inventoried as a single collection. Information about each photograph, including location, description, and mission, are in the document_database in ganymede_diagram_database.pdf and ganymede_photo_database.pdf. The photographs and documentation are from the Dr. Ronald Greeley archive at the Arizona State University Ronald Greeley Center for Planetary Studies, Tempe, Arizona. -
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Saturn Zonal Winds Observarions Collection
Saturn's zonal wind profile in 2004-2009 from Cassini ISS images -
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Huygens Descent Imager/Spectral Radiometer data_raw collection file
Raw Data Products data collection for the Huygens DISR PDS4 bundle. -
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data collection for the "GASKELL MIMAS SHAPE MODEL" bundle
This is the data collection for the gaskell.mimas.shape-model bundle. The shape model of Mimas derived by Robert Gaskell from Cassini ISSNA and ISSWA images and Voyager 1 ISSN images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on June 26, 2012. Vertex-facet versions of the models are also provided. -
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Mars Target Encyclopedia MPF Collection
MPF collection for the Mars Target Encyclopedia bundle -
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MER2 Pancam Raw Data Collection
This collection contains raw images from the Panoramic Cameras (Pancam) on the Mars Exploration Rover 2 (Spirit). These products were produced by the Pancam Science Team. -
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Whiteley NEO Photometry V1.0
This data set includes the ECAS system (Eight Color Asteroid Survey) photometry and taxonomic types of 77 Near Earth Objects published by R.J. Whiteley in his thesis (Whiteley, 2001. A compositional and dynamical survey of the near-earth asteroids. Ph.D. thesis, University of Hawaii), [WHITELEY2001] The ECAS system is established in Zellner et al. 1985, Icarus 61, 355-416 [ZELLNERETAL1985]. The original ECAS survey is available in PDS as data set EAR-A-2CP-3-RDR-ECAS-V3.0. The data presented here are new measurements based on the ECAS system. -
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MER1 Microscopic Imager Raw Data Collection
This collection contains raw images from the Microscopic Imager (MI) on the Mars Exploration Rover 1 (Opportunity). These products were produced by the MI Science Team. -
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MER1 Microscopic Imager Calibrated Data Collection
This collection contains calibrated images from the Microscopic Imager (MI) on the Mars Exploration Rover 1 (Opportunity). These products were produced by the MI Science Team. -
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data collection for the "EROS MSI IMAGES WITH GEOMETRY BACKPLANES " bundle
This is the data collection for the nearmsi.shapebackplane bundle. This data set contains data products for 93,397 images obtained by the Multi-Spectral Imager (MSI) of the Near Earth Asteroid Rendezvous (NEAR) mission during the orbital phase at asteroid 433 Eros. The data products include geometric and geophysical information for each pixel. The data products are in the form of backplanes, stored in the FITS image format. There is one backplane file for each MSI image. Each of the MSI backplane files is a 16-band image cube. The bands of the cube contain the information detailed below calculated for the center of each pixel: 1: Pixel values (I/F) of the original FITS images delivered to the PDS by the NEAR team [Murchie et al., 2001], linearly resampled to rectify the image by squaring the pixels. The original image size is 537 x 244 pixels and the rectified size is 537 x 412 pixels. 2: x coordinate (kilometers) of the intercept with the surface of the asteroid in body-fixed reference frame 3: y coordinate (kilometers) of the intercept with the surface of the asteroid in body-fixed reference frame 4: z coordinate (kilometers) of the intercept with the surface of the asteroid in body-fixed reference frame 5: latitude (planetocentric, degrees) 6: longitude (degrees east) 7: radial distance (kilometers) from the asteroid center of figure 8: solar incidence angle (degrees) 9: emission angle (degrees) 10: solar phase angle (degrees) 11: horizontal pixel scale (kilometers) 12: vertical pixel scale (kilometers) 13: average surface slope relative to gravity (degrees) 14: average elevation relative to gravity (meters) 15: average gravitational acceleration (meters/[s^2]) 16: average gravitational potential (J/kg) -
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Small Body Optical Shape Models V1.0
The Small Body Shape Models data set contains the Peter Thomas shape models for small solar system bodies, as well as image mosaics constructed from these models. These shape models are based upon optical data from a variety of spacecraft instruments, including the Galileo SSI, NEAR MSI, Viking orbiter, Voyager 1 & 2, and the Hubble Space Telescope. The data has been published in a variety of publications between 1984 and 1999. -
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Visual Imaging and Photometry of (29981) 1999 TD10 V2.0
The outer solar system object (29981) 1999 TD10 was observed in the R band in September 2001, and in B, V, R, and I in October 2002. We derive B-V=0.80+/-0.05mag, V-R=0.48+/-0.05mag, and R-I=0.44+/-0.05mag. Combining our data with the data from Rousselot et. al. 2003, we derive a synodic period of 15.382+/-0.001hr in agreement with the period from Rousselot et. al. 2003. Our observations show no evidence of a coma. -
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MER1 Pancam Photometry Data Collection
MER1 Pancam Photometry Data Collection -
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MER2 Pancam Calibrated Data Collection
This collection contains calibrated images from the Panoramic Cameras (Pancam) on the Mars Exploration Rover 2 (Spirit). These products were produced by the Pancam Science Team. -
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Saturn Small Moon Shape Models V1.0
Digital shape models have been constructed from Cassini Imaging Science Subsystem (ISS) data for eleven of the small satellites of Saturn and delivered to the Planetary Data System. These satellites are: Pan, Daphnis, Atlas, Prometheus, Pandora, Epimetheus, Janus, Telesto, Calypso, Helene, and Hyperion. These models typically have uncertainties well under 0.5 km. They are appropriate for global geometric, geologic, and geophysical studies, and regional slope and topography study. They are useful in studying morphologies of only the relatively largest-sized craters. Studies based on early versions of these shape models are in Thomas et al., 2013 -
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EPOXI MRI-VIS 103P/Hartley 2 Encounter Photometry Collection
We perform photometric measurements of comet 103P/Hartley 2 using images taken through the CLEAR1 (broadband, 200-1100 nm), CN (387 nm), OH (309 nm), C2 (514 nm), and two continuum filters (Ultraviolet at 345 nm and Green at 526 nm) of the Medium Resolution Instrument (MRI) on board the Deep Impact flyby spacecraft from 1 October to 26 November 2010 during the EPOXI mission. -
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Mars Global Cave Candidate Catalog
Mars Global Cave Candidate Catalog -
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data collection for the "SDSS-BASED ASTEROID TAXONOMY" bundle
This is the data collection for the ast.sdss-based-taxonomy bundle. The Sloan Digital Sky Survey Moving Object Catalog (SDSS-MOC) is a large data set that provides five-filter magnitudes and astrometric information for all moving objects identified in the SDSS images (Izevic et al., 2010). The photometric observations were classified by Carvano et al. (2010) into nine taxonomic classes: Vp, Op, Qp, Sp, Ap, Lp, Dp, Xp and Cp, which are related to the classes and complexes of Bus Taxonomy (Bus & Binzel, 2002b). This data set is contains the taxonomic classification of each SDSS detections and its compilation for each observed asteroid. -
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Nathair Facula Topography and Photometric Cube Data V1.0
This bundle contains regional topography and photometric data for two locations within Nathair Facula, Mercury. Both locations focus on volcanic vents and pyroclastic deposits near 35.86 Lat 63.93 E Lon. The data was generated using the Gaskell Stereophotoclinometry (SPC) software suite with images from the MESSENGER mission to Mercury. In addition to the topographic heights of the Digital Terrain Model (DTM), photometric data is aligned to and has the same horizontal spacing as the topographic data. For select Mercury Dual Imaging System (MDIS) Narrow Angle Camera (NAC) or Wide Angle Camera (WAC) images, four photometric data products are available; I/F (reflectance), Local Phase Angle, Local Emission Angle, and Local Incidence Angle. One DTM represents heights every 120 m and has a size of 130 by 130 km, while the other represents heights every 60 m and has a size of 80 by 80 km. The two DTMs partially overlap. -
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MER1 Pancam Derived Opacity Data Collection
This collection contains atmospheric opacity data derived from the Panoramic Cameras (Pancam) on the Mars Exploration Rovers. These products were produced by the Pancam Science Team. -
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Huygens Descent Imager/Spectral Radiometer Document collection file
Document Products data collection for the Huygens DISR PDS4 bundle. -
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Mars Global Cave Candidate Catalog
Mars Global Cave Candidate Catalog -
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LCROSS Near Infrared Camera 1 Data Collection
This collection contains data products for the Near Infrared Camera 1 instrument of the LCROSS spacecraft. -
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Cassini ISS Global Maps of Jupiter and Saturn Derived Data Collection
Cassini ISS Global Maps of Jupiter and Saturn -
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Saturn Small Moon Shape Models V1.0
Digital shape models have been constructed from Cassini Imaging Science Subsystem (ISS) data for eleven of the small satellites of Saturn and delivered to the Planetary Data System. These satellites are: Pan, Daphnis, Atlas, Prometheus, Pandora, Epimetheus, Janus, Telesto, Calypso, Helene, and Hyperion. These models typically have uncertainties well under 0.5 km. They are appropriate for global geometric, geologic, and geophysical studies, and regional slope and topography study. They are useful in studying morphologies of only the relatively largest-sized craters. Studies based on early versions of these shape models are in Thomas et al., 2013 -
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New Horizons KEM1 Encounter Multispectral Visible Imaging Camera (MVIC) Partially Processed Data
This data set contains partially processed data taken by the New Horizons Multispectral Visible Imaging Camera (MVIC) instrument during the KEM1 ENCOUNTER mission phase. This version includes data acquired by the spacecraft between 08/14/2018 and 04/30/2022. It only includes data downlinked before 05/01/2022. The data includes functional tests and images during the approach and departure of Arrokoth. A look back at Pluto was also performed after the Arrokoth flyby. A Color Scan of Neptune and Uranus was done along with a Solar Star Calibration and Radiometric Calibration. These data were migrated from the PDS3 dataset: NH-A-MVIC-3-KEM1-V6.0. -
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Phoebe SPC Shape Model and Assessment Products V1.0
This bundle contains a shape model for the Saturnian moon Phoebe, along with quality assessment data. The global model is similar to the previously archived "Gaskell Phoebe Shape Model", but is provided in multiple formats. -
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data collection for the "NEAR-INFRARED PHOTOMETRY OF ASTEROIDS FROM DENIS" bundle
This is the data collection for the gbo.ast.denis.ir-photometry bundle. The DENIS program (Deep European Near-Infrared southern sky Survey) was a ground-based survey of the southern sky with the aim of providing an extensive I,J,Ks photometric catalog of point and extended sources. It was carried out at the 1.0 meter ESO telescope at La Silla, Chile from late 1995 through the end of 1999. This data set contains the DENIS I,J,Ks photometry for 2000 known asteroids identified in the DENIS catalog. -
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Mars Target Encyclopedia MER-1 Collection
MER-1 collection for the Mars Target Encyclopedia bundle -
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Small Body Optical Shape Models V1.0
The Small Body Shape Models data set contains the Peter Thomas shape models for small solar system bodies, as well as image mosaics constructed from these models. These shape models are based upon optical data from a variety of spacecraft instruments, including the Galileo SSI, NEAR MSI, Viking orbiter, Voyager 1 & 2, and the Hubble Space Telescope. The data has been published in a variety of publications between 1984 and 1999. -
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Whiteley NEO Photometry V1.0
This data set includes the ECAS system (Eight Color Asteroid Survey) photometry and taxonomic types of 77 Near Earth Objects published by R.J. Whiteley in his thesis (Whiteley, 2001. A compositional and dynamical survey of the near-earth asteroids. Ph.D. thesis, University of Hawaii), [WHITELEY2001] The ECAS system is established in Zellner et al. 1985, Icarus 61, 355-416 [ZELLNERETAL1985]. The original ECAS survey is available in PDS as data set EAR-A-2CP-3-RDR-ECAS-V3.0. The data presented here are new measurements based on the ECAS system. -
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data collection for the "SDSS MOVING OBJECT CATALOG" bundle
This is the data collection for the gbo.sdss-moc.phot bundle. The Sloan Digital Sky Survey (SDSS) Moving Object Catalog 4th release lists astrometric and photometric data for moving objects detected in the SDSS. The catalog includes various identification parameters, SDSS astrometric measurements (five SDSS magnitudes and their errors), and orbital elements for previously cataloged asteroids. The data set also includes a list of the runs from which data are included, and filter response curves. -
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LCROSS Near Infrared Camera 2 Data Collection
This collection contains data products for the Near Infrared Camera 2 instrument of the LCROSS spacecraft. -
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MER1 Pancam Raw Data Collection
This collection contains raw images from the Panoramic Cameras (Pancam) on the Mars Exploration Rover 1 (Opportunity). These products were produced by the Pancam Science Team. -
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Lunar Topography and Photometric Cube Data V1.0
This package contains topography and photometric data generated by the Gaskell Stereophotoclinometry (SPC) software suite. It focuses on six regions on the Moon. These include wrinkle ridges at Dorsa Aldrovandi, two locations of the lunar swirl within Mare Ingenii, Karpinskiy crater, a swirl within Mare Moscoviense, Reiner Gamma, and Tsiolkovskiy crater. We generated regional Digital Terrain Models (DTM), each about 50 to 100 square kilometers, using Lunar Reconnaissance Orbiter (LRO) Narrow Angle Camera (NAC) images from both the right and left cameras. Depending on the location, each vertex of the topography represents heights every 5 to 0.7 meters, with an uncertainty of about one to two vertices. The topography data is provided in both cubes readable by the USGS ISIS program, and as a geoTIFF which can be read by programs such as ArcGIS. We generated photometric data (in cube format) that is aligned to, and has the same horizontal spacing as, the topographic cube data. For each LROC image, four cubes were generated; I/F (reflectance), Local Phase Angle, Local Emission Angle, and Local Incidence Angle. Each cube pixel represents the value at each vertex of the DTM. -
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data collection for the "GASKELL TETHYS SHAPE MODEL" bundle
This is the data collection for the gaskell.tethys.shape-model bundle. The shape model of Tethys derived by Robert Gaskell from Cassini Imaging Science Subsystem narrow and wide angle camera (ISSNA and ISSWA) images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on July 25, 2012. Vertex-facet versions of the models are also provided. -
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Raw Data Collection for the Cassini ISS Observations from the Cruise to Saturn
This is the collection of raw ISS images and associated metadata from the Cassini cruise to Saturn. -
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HST images, albedo maps, and shape of (1) Ceres V1.0
This dataset contains 267 HST ACS/HRC images of asteroid (1) Ceres obtained in 2003/2004 at three wavelengths, 535 nm, 335 nm, and 223 nm. They have been photometrically calibrated to standard reflectance unit I/F. The dataset also includes a shape for Ceres, as well as three surface albedo maps covering the area between +/-50 deg latitude, derived from these images. -
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Mars Global Cave Candidate Catalog
Mars Global Cave Candidate Catalog -
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HST images, albedo maps, and shape of (1) Ceres V1.0
This dataset contains 267 HST ACS/HRC images of asteroid (1) Ceres obtained in 2003/2004 at three wavelengths, 535 nm, 335 nm, and 223 nm. They have been photometrically calibrated to standard reflectance unit I/F. The dataset also includes a shape for Ceres, as well as three surface albedo maps covering the area between +/-50 deg latitude, derived from these images. -
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MER2 Pancam Derived Color Data Collection
This collection contains color mosaics from the Panoramic Cameras (Pancam) on the Mars Exploration Rover 2 (Opportunity). These products were produced by the Pancam Science Team. -
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Roberts Eros Ponds Catalog V1.1
This data set contains two tables describing the size and location of ponded deposits on asteroid 433 Eros. Both tables contain the same pond information, but one is presented in the format required for ingestion by a publicly available 3D visualization application, the Small Body Mapping Tool (Ernst et al., 2018; http://sbmt.jhuapl.edu). -
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HST UV Slitless Reflectance Spectra of (1) Ceres V1.0
This archive package contains the reflectance spectra of Ceres from 121 nm to 198 nm based on the slitless spectrographic observations using HST/ACS SBC performed on 2007 November 25. Ceres was spatially resolved to about 21 pixels in diameter. The raw spectra were extracted from the raw 2D spectral image corresponding to all pixels within the disk of Ceres, calibrated to intensity unit and then to reflectance unit. The final reflectance spectra of Ceres is the average of all spectra over the whole disk of Ceres. All intermediate data and the final average reflectance spectra are included in the data set.
Data Sets and Information
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